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In the era of Chandra and XMM-Newton, the detection (or nondetection) ofdiffuse and/or point-like X-ray sources within planetary nebulae (PNe) yieldsimportant, unique insight into PN shaping processes. Diffuse X-ray sources,whether due to ``hot bubbles'' or to collimated outflows or jets, allow us toprobe the energetic shocks within PN wind interaction regions. Meanwhile, X-raypoint sources provide potential diagnostics of magnetic fields, accretiondisks, and/or binary companions at PN cores. Here, I highlight recent X-rayobservational results and trends that have the potential to shed new light onthe origin and evolution of the structure of PNe.

X-ray Emission from Planetary Nebulae and their Central Stars: a Status Report